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相关论文: X-Ray Spectral Model from Clumpy Torus and Its App…

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Circinus galaxy is a nearby composite starburst/AGN system. In this work we re-analyze the GeV emission from Circinus with 10 years of {\it Fermi}-LAT Pass 8 data. In the energy range of 1-500 GeV, the spectrum can be well fitted by a…

高能天体物理现象 · 物理学 2020-01-08 Xiao-Lei Guo , Yu-Liang Xin , Neng-Hui Liao , Yi-Zhong Fan

Near- and mid-infrared interferometers have resolved the dusty parsec-scale obscurer (torus) around nearby active galactic nuclei (AGNs). With the arrival of extremely large single-aperture telescopes, the emission morphology will soon be…

星系天体物理 · 物理学 2021-10-13 R. Nikutta , E. Lopez-Rodriguez , K. Ichikawa , N. A. Levenson , C. Packham , S. F. Hönig , A. Alonso-Herrero

We have analyzed spectra for all active galactic nuclei in the Rossi X-ray Timing Explorer (RXTE) archive. We present long-term average values of absorption, Fe line equivalent width, Compton reflection and photon index, as well as…

高能天体物理现象 · 物理学 2015-06-16 Elizabeth Rivers , Alex Markowitz , Richard Rothschild

We present a detailed spectral analysis of point-like X-ray sources in the XMM-COSMOS field. Our sample of 135 sources only includes those that have more than 100 net counts in the 0.3-10 keV energy band and have been identified through…

We present spectral analysis of the Crab Nebula obtained with the {\it Chandra} X-ray observatory. The X-ray spectrum is characterized by a power-law whose index varies across the nebula. The variation can be discussed in terms of the…

天体物理学 · 物理学 2009-11-10 K. Mori , D. N. Burrows , J. J. Hester , G. G. Pavlov , S. Shibata , H. Tsunemi

We present 31.5 micron imaging photometry of 11 nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy (SOFIA) using the Faint Object infraRed CAmera for the SOFIA Telescope (FORCAST). We tentatively…

A subparsec-scale dense plasma torus around an active galactic nucleus (AGN) is unveiled. We report on very-long-baseline interferometry (VLBI) observations at 2.3, 8.4, and 15.4 GHz towards the active galaxy NGC 1052. The convex spectra of…

天体物理学 · 物理学 2015-06-24 S. Kameno , S. Sawada-Satoh , M. Inoue , Z. -Q. Shen , K. Wajima

High quality 4500-6800 A spectropolarimetric observations of the Circinus galaxy are reported. These show polarized and relatively broad (FWHM~3300 km/s) Halpha (as well as marginal Hbeta) arising from a <3" (<60 pc) region centered on the…

天体物理学 · 物理学 2007-05-23 E. Oliva , A. Marconi , A. Cimatti , S. di Serego Alighieri

Aims: The unification scheme of Seyfert galaxies predicts that the observed differences between type 1 and type 2 Seyfert galaxies are solely due to the differing orientations of the toroidal-shaped obscuring material around AGN. The…

高能天体物理现象 · 物理学 2015-03-17 Veeresh Singh , Prajval Shastri , Guido Risaliti

Circinus X-1 is a neutron-star-accreting X-ray binary in a wide (P$_{\rm orb}$ = 16.6 d), eccentric orbit. After two years of relatively low X-ray luminosity, in May 2010 Circinus X-1 went into outburst, reaching 0.4 Crab flux. This…

高能天体物理现象 · 物理学 2015-06-04 A. D'Aì , E. Bozzo , A. Papitto , R. Iaria , T. Di Salvo , L. Burderi , A. Riggio , E. Egron , N. R. Robba

The Imaging X-ray Polarimetry Explorer (IXPE) detected X-ray polarization in the nearest Seyfert 2 galaxy, the Circinus galaxy, for the first time. To reproduce the IXPE results, we computed the degree of polarization based on two types of…

高能天体物理现象 · 物理学 2023-10-31 Atsushi Tanimoto , Keiichi Wada , Yuki Kudoh , Hirokazu Odaka , Ryosuke Uematsu , Shoji Ogawa

We present the broadband (0.5-100 keV) spectra of three heavily obscured Active Galactic Nuclei (AGNs), NGC 1106, UGC 03752, and NGC 2788A, observed with Suzaku and Swift/Burst Alert Telescope (BAT). The targets are selected from the…

星系天体物理 · 物理学 2016-03-23 Atsushi Tanimoto , Yoshihiro Ueda , Taiki Kawamuro , Claudio Ricci

We investigated the gravitational microlensing of active galactic nucleus dusty tori in the case of lensed quasars in the infrared domain. The dusty torus is modeled as a clumpy two-phase medium. To obtain spectral energy distributions and…

宇宙学与河外天体物理 · 物理学 2012-09-04 Marko Stalevski , Predrag Jovanović , Luka Č. Popović , Maarten Baes

We present an exhaustive methodology for fitting Compton-thick X-ray reprocessor models to obscured AGNs and for interpreting the results. We focus on the MYTORUS model but also utilize other models. We apply the techniques to Suzaku,…

高能天体物理现象 · 物理学 2015-06-04 Tahir Yaqoob

Current X-ray missions are providing high-quality X-ray spectra from neutron stars (NSs) in quiescent low-mass X-ray binaries (qLMXBs). This has motivated us to calculate new hydrogen-atmosphere models, including opacity due to free-free…

天体物理学 · 物理学 2009-11-13 Craig O. Heinke , George B. Rybicki , Ramesh Narayan , Jonathan E. Grindlay

We have analyzed a Suzaku long-look of the active galactic nucleus MCG-2-58-22, a type 1.5 Seyfert with very little X-ray absorption in the line of sight and prominent features arising from reflection off circumnuclear material: the Fe line…

宇宙学与河外天体物理 · 物理学 2015-05-28 Elizabeth Rivers , Alex Markowitz , Richard Rothschild

Context: We investigate mid-infrared and X-ray properties of the dusty torus invoked in the unification scenario for active galactic nuclei. Aims: We use the relation between mid IR and hard X-ray luminosities to constrain the geometry and…

天体物理学 · 物理学 2009-11-13 Hannes Horst , Poshak Gandhi , Alain Smette , Wolfgang J. Duschl

In this paper, we estimate the gamma-ray and neutrino fluxes coming from dark matter annihilation in a Milky Way framework provided by a recent N-BODY HORIZON simulation. We first study the characteristics of the simulation and highlight…

天体物理学 · 物理学 2009-06-23 E. Athanassoula , F. -S. Ling , E. Nezri , R. Teyssier

We present the hard X-ray (20-100 keV) observations of Cygnus X-1 obtained using a large area balloon-borne Xenon filled Multi-anode Proportional Counter (XMPC) telescope. The observations were carried out during the gamma_2 state of the…

天体物理学 · 物理学 2007-05-23 V. R. Chitnis , A. R. Rao , P. C. Agrawal

Using the X-ray-selected active galactic nuclei (AGN) from the XMM-XXL north survey and the SDSS Baryon Oscillation Spectroscopic Survey (BOSS) spectroscopic follow-up of them, we compare the properties of X-ray unobscured and obscured…